Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0

This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process.

Data and Resources

This dataset has no data

Additional Info

Field Value
Maintainer Thomas Morgan
Last Updated July 17, 2025, 17:02 (UTC)
Created March 31, 2025, 23:47 (UTC)
accessLevel public
accrualPeriodicity irregular
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harvest_object_id 059698cc-49db-4810-b29c-7ae570560049
harvest_source_id 61638e72-b36c-4866-9d28-551a3062f158
harvest_source_title DNG Legacy Data
identifier urn:nasa:pds:gbo.ast.smass2.spectra
issued 2021-05-21
landingPage https://pds.nasa.gov/ds-view/pds/viewBundle.jsp?identifier=urn%3Anasa%3Apds%3Agbo.ast.smass2.spectra&version=1.0
license http://www.usa.gov/publicdomain/label/1.0/
modified 2021-05-21
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publisher National Aeronautics and Space Administration
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